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Similar to Near-Earth Objects EPS Conference 250914
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Near-Earth Objects EPS Conference 250914
- 1. Imagecredit:ESA Facing up to the risks of impacts of Near- Earth Objects Debbie Lewis MSc FEPS
- 2. We may never encounter a natural disaster more violent than a storm. And so we become complacent, relaxed, unconcerned. But in the history of nature, the record is clear. Worlds have been devastated. On the landscapes of other planets where the records of the past have been preserved, there is abundant evidence of major catastrophes. Even on the Earth, even in our own century, bizarre natural events have occurred (Sagan, 1981:92).
- 3. • What is the hazard? • Sample cases • What is everybody doing? • What is ESA doing? • Conclusions/questions Outline Meteorite (10 cm)
- 4. • Near-Earth Object (NEO): Any asteroid coming closer than 0.3 AU to the Earth • 1 AU = Astronomical Unit = distance Sun-Earth = 149.6 Mio km • Threatening object: Any asteroid that may hit the Earth • Risk list: A list containing all threatening objects Definitions/terminology 500 m NEO Itokawa (credit: JAXA)
- 5. Known number of Near Earth Asteroids
- 6. Near Earth Objects population (From JPL – NEO site)
- 7. Estimated Number of Asteroids and NEOs (Data from NEODyS or JPL NEO site, Aug 2013) • > 600 000 known Asteroids • > 10 000 known NEOs • > 400 NEOs in risk list (NEOs with small but non-zero impact probability within next 100 years) • Estimated number of known NEOs: – 90% of NEOs with diameter larger than 1 km (≥ 860 NEAs + 94 near-Earth Comets of a total of ≈ 1050) – 15-25% of NEOs larger than 140 m (total ≈ 20,000 - 30,000) – < 2.0% of NEOs larger than 30 m (total ≈ 500,000 - 1,000,000) Most NEOs are still unknown!
- 9. NEO impacts: frequency and effects • Asteroids (and Comets) hit Earth with very high velocities. • typical: 10 - 20 km/s, 20 times faster than a gun bullet! NEO diameter Impact energy [Megatons TNT] (1g TNT ≡ 4184 J) Typical interval [Years] Effect 2 mm 1 per hour (visible for each location) Nice meteor 3 m 0.002 1 Fireball, Sudan Event, Meteorites reach ground 10 m 0.08 10 Big fireball, fear, shock wave, 5- fold energy of Hiroshima bomb 40 m 5 500 Tunguska explosion or Crater 140 m 220 10,000 Regional destruction, Tsunami 500 m 10,000 200,000 Europe-wide destruction 1 km 80,000 700,000 Millions dead, global effects 10 km 80 million 100 million End of human civilisation
- 10. Age (years) or date Impactor Size Location Consequences 1 K-T mass biota boundary between Cretaceous and tertiary geological periods 65 Million years ago 10-15km diameter asteroid or comet 200km crater discovered Chicxulub, Pueblo Yucatan Peninsula Gulf of Mexico Estimate extinction of 70% of animal and plant species. Penetrative tsunamis. Cessation of photosynthesis and climatic cooling 2 50,000 years ago Meteorite 150 ft in diameter Barringer Crater Arizona Creation of a crater 1 mile across, 2.4 miles in circumference and >550 ft in depth 3 4,000 years ago Meteorite Kaali Crater, Estonia Formation of 100 m crater NEO impacts: frequency and effects
- 11. Tunguska 30 June 1908 - 105 years ago 2000 km2 of Taiga were destroyed in Siberia
- 13. Carancas, Peru Crater with 14-m diameter formed by impact from space in 2007.
- 14. Chelyabinsk Impact Event • Location: 55.2o N, 61.4o E (near Chelyabinsk, Russia) • Date/time: 15 Feb 2013, 03:20 UT (09:20 LT) • Diameter of object: 19 m, mass ≈ 12000 t • Entry velocity: 18.6 km/s, entry angle: 20o from surface • Total energy: equiv. to 480 kt TNT • Altitude of main explosion: 30 – 25 km • Max brightness of fireball: m ≈ -30 (about 30 x sun brightness) • 7300 buildings damaged • > 1500 people injured • > 100 kg of meteorites found (usually small pieces, asteroid was ordinary chondrite) • Asteroid could not be seen approaching (too close to sun direct.) and was too faint for prior detection during the last 10 years
- 15. Uncertainty Uncertainty exists as to the extent of the scale of a NEO impact for six reasons: 1. The NEO population is not sufficiently understood 2. Inability to determine impact levels for objects between 50m and 140m in diameter 3. Unknown composition of NEOs 4. Variable collision effects 5. Effects may exceed local and regional areas and have global effects 6. The size and type of NEO which would cause these effects
- 16. Risk Treatment Four risk treatment methods have been identified to mitigate the NEO hazard: •Characterisation •Civil protection •Planetary defence •Establishment of a research programme
- 17. Current State of Preparedness • Kinetic Impactor • Gravity Tractor • Nuclear Device • Civil Protection
- 19. Discussions Within UN COPUOS • Action Team 14 of UN COPUOS has developed a response strategy • Adopted in Jun 2013 • Two groups are to be installed: – International Asteroid Warning Network (includes interface to emergency response) – Space Missions Planning Advisory Group
- 20. Extant Guidance - UN System • Increasing public awareness • Obtaining commitment from public authorities • Stimulating interdisciplinary and inter-sector partnership and expanding risk-reduction networking at all levels • Enhancing scientific research of the causes of natural disasters and the effects of natural hazards and related technological and environmental disasters on societies
- 22. NEO Coordination Centre – ESRIN, Italy SSA-NEO Coordination Centre - inaugurated 22 May 2013
- 23. The SSA-NEO web portal • Federates some key European assets: – NEODyS = orbit computation, prediction, risk list – Physical properties database – Priority list = showing objects in need of observations http://neo.ssa.esa.int
- 24. 2015 IAA Planetary Defense Conference: Assessing Impact Risk & Managing Response April 13-17th 2015 Frascati, Italy http://www.pdc2015.org/